"Cosmos" is just another word for universe, and "cosmology" is the study of the origin, evolution and fate of the universe. Some of the best minds in history - both philosophers and
scientists - have applied themselves to an understanding of just what the universe is and where it came from, suggesting in the process a bewildering variety of theories and ideas, from the Cosmic
Egg to the Big Bang and beyond. Here are some of the main ones, in approximate chronological order:

• Brahmanda (Cosmic Egg) Universe - The Hindu Rigveda, written in India around the 15th - 12th Century B.C., describes a cyclical or oscillating universe in which a
“cosmic egg”, or Brahmanda, containing the whole universe (including the Sun, Moon, planets and all of space) expands out of a single concentrated point called a Bindu before subsequently
collapsing again. The universe cycles infinitely between expansion and total collapse.

• Anaxagorian Universe - The 5th Century B.C. Greek philosopher Anaxagoras believed that the original state of the cosmos was a primordial mixture of all its ingredients
which existed in infinitesimally small fragments of themselves. This mixture was not entirely uniform, and some ingredients were present in higher concentrations than others, as well as varying from
place to place. At some point in time, this mixture was set in motion by the action of “nous” (mind), and the whirling motion shifted and separated out the ingredients, ultimately producing the
cosmos of separate material objects, all with different properties, that we see today.

• Atomist Universe - Later in the 5th Century B.C., the Greek philosophers Leucippus and Democritus founded the school of Atomism, which held that the universe was composed
of very small, indivisible and indestructible building blocks known as atoms (from the Greek “atomos”, meaning “uncuttable”). All of reality and all the objects in the universe is composed of
different arrangements of these eternal atoms and an infinite void, in which they form different combinations and shapes.

Aristotelian Universe - The Greek philosopher Aristotle, in the 4th Century B.C., established a geocentric universe in which the fixed, spherical Earth is at the centre, surrounded by
concentric celestial planets and stars. Although he believed the universe to be finite in size, he stressed that it exists unchanged and static throughout eternity. Aristotle definitively
established the four classical elemnts of fire, air, earth and water. He later added a fifth element Aether, to describe the void that fills the universe above the terrestrial Earth.

• Stoic Universe - The Stoic philosophers of ancient Greece (3rd Century B.C. and after) believed in a kind of island universe in which a finite cosmos is surrounded by
an infinite void (not dissimilar in principle to a galaxy). They held that the cosmos is in a constant state of flux, and pulsates in size and periodically passes through upheavals and
conflagrations. In the Stoic view, the universe is like a giant living body, with its leading part being the stars and the Sun, but in which all parts are interconnected, so that what happens in one
place affects what happens elsewhere. They also held a cyclical view of history, in which the world was once pure fire and would become fire again (an idea borrowed from Heraclitus).

The Beggining of Heliocentric Theory

• Heliocentric Universe – It is claimed that in 3rd Century B.C. Greek astronomer and mathematician Aristarchus of Samos was the first to present an explicit argument for
a heliocentric model of the Solar System, placing the Sun, not the Earth, at the centre of the known universe. His ideas apparently were rejected in favour of the geocentric theories of
Aristotle and Ptolemy until they were successfully revived nearly 1800 years later! by Copernicus. However, there were exceptions: Heliocentics also claim that Seleucus of Seleucia, who lived
about a century after Aristarchus, supported his theories and used the tides to explain heliocentricity and the influence of the Moon; the Indian astronomer and mathematician Aryabhata described
elliptical orbits around the Sun at the end of of the 5th Century A.D.; as did the Muslim astronomer Ja'far ibn Muhammad Abu Ma'shar al-Balkhi in the 9th Century.

• Ptolemaic Universe - The 2nd Century A.D. Roman-Egyptian mathematician and astronomer Ptolemy (Claudius Ptolemaeus) described a geocentric model largely based on
Aristotelian ideas, in which the planets and the rest of the universe orbit about a stationary Earth in circular epicycles. In terms of longevity, it was perhaps the most successful cosmological
model of all time. Modifications to the basic Ptolemaic system were suggested by the Islamic Maragha School in the 13th, 14th and 15th Centuries including the first accurate lunar model by Ibn
al-Shatir, and the rejection of a stationery Earth in favour of a rotating Earth by Ali Qushji.

• Abrahamic Universe - Several medieval Christian, Muslim and Jewish scholars put forward the idea of a universe which was finite in time. In the 6th Century A.D., the
Christian philospher John Philoponus of Alexandria argued against the ancient Greek notion of an infinite past, and was perhaps the first commentator to argue that the universe is finite in time and
therefore had a beginning. Early Muslim theologians such as Al-Kindi (9th Century) and Al-Ghazali (11th Century) offered logical arguments supporting a finite universe, as did the 10th Century Jewish
philosopher Saadia Gaon.

• Partially Heliocentric Universe - In the 15th and early 16th Century, Somayaji Nilakantha of the Kerala school of astronomy and mathematics in southern India developed a
computational system for a partially heliocentric planetary model in which Mercury, Venus, Mars, Jupiter and Saturn orbited the Sun, which in turn orbited the Earth. This was very similar to the
Tychonic system proposed by the Danish nobleman Tycho Brahe later in the 16th Century as a kind of hybrid of the Ptolemaic and Copernican models.

• Copernican Universe - In 1543, the Polish astronomer and polymath Nicolaus Copernicus adapted the geocentric Maragha model of Ibn al-Shatir to meet the requirements of
the ancient heliocentric universe of Aristarchus. His publication of a scientific theory of heliocentrism, demonstrating that the motions of celestial objects can be explained without putting the
Earth at rest in the centre of the universe, stimulated further scientific investigations and became a landmark in the history of modern science, sometimes known as the Copernican Revolution. His
Copernican Principle (that the Earth is not in a central, specially favoured position) and its implication that celestial bodies obey physical laws identical to those on Earth, first established
cosmology as a science rather than a branch of metaphysics. In 1576, the English astronomer Thomas Digges popularized Copernicus’ ideas and also extended them by positing the existence of a multitude
of stars extending to infinity, rather than just Copernicus’ narrow band of fixed stars.

• The Italian philosopher Giordano Bruno took the Copernican Principle a stage further in 1584 by suggesting that even the Solar System is not the centre of the universe,
but rather a relatively insignificant star system among an infinite multitude of others. In 1605, Johannes Kepler made further refinements by finally abandoning the classical assumption of circular
orbits in favour of elliptical orbits which could explain the strange apparent movements of the planets. Galileo's controversial support of Copernicus' heliocentric model in the early 17th Century
was denounced by the Inquisition but nevertheless helped to popularize the idea.

• Cartesian Vortex Universe - In the mid-17th Century, the French philosopher René Descartes outlined a model of the universe with many of the characteristics of Newton’s
later static, infinite universe. But, according to Descartes, the vacuum of space was not empty at all, but was filled with matter that swirled around in large and small vortices. His model involved
a system of huge swirling whirlpools of ethereal or fine matter, producing what would later be called gravitational effects.

• Static (or Newtonian) Universe - In 1687, Sir Isaac Newton published his “Principia”, which described, among other things, a static, steady state, infinite universe which
even Einstein, in the early 20th Century, took as a given (at least until events proved otherwise). Hierarchical Universe and the Nebular Hypothesis - Although still generally based on a Newtonian
static universe, the matter in a hierarchical universe is clustered on ever larger scales of hierarchy, and is endlessly being recycled. It was first proposed in 1734 by the Swedish scientist and
philosopher Emanuel Swedenborg, and developed further (independently) by Thomas Wright (1750), Immanuel Kant (1755) and Johann Heinrich Lambert (1761), and a similar model was proposed in 1796 by the
Frenchman Pierre-Simon Laplace.

Einsteinian Universe - The model of the universe assumed by Albert Einstein in his groundbreaking theory of gravity in the early 20th Century was not dissimilar to Newton’s in that it was
a static, dynamically stable universe which was neither expanding nor contracting. However, he had to add in a “cosmological constant” to his general relativity equations to counteract the dynamical
effects of gravity which would otherwise have caused the universe to collapse in on itself (although he later abandoned that part of his theory when Edwin Hubbler definitively showed in 1929 that the
universe was not in fact static).

• Big Bang Model of the Universe – After Hubbles demonstration of the continuously expanding in 1929 (and especially after the discovery of cosmic background radiation by
Arno Penzias and Robert Wilson in 1965), some version of the Big Bang theory has generally been the mainstream scientific view. The theory describes the universe as originating in an infinitely
tiny, infinitely dense point (or singularity) between 13 and 14 billion years ago, from where it has been expanding ever since. The essential statement of the theory is usually attributed to the
Belgian Roman Catholic priest and physicist Georges Lemaitre in 1927 (even before Hubble corroborating evidence), although a similar theory had been proposed, although not pursued, 1922 by the
Russian Alexander Friedmann in 1922. Friedmann actually developed two models of an expanding universe based on Einstein’s General Relitivity equations, one with positive curvature or spherical space,
and one with negative curvature or hyperbolic space.

• Oscillating Universe - This was Einsteins favoured model after he rejected his own original model in the 1930s. The oscillating universe followed from Alexander
Friedmann’s model of an expanding universe based on general relitivity equations for a universe with positive curvature (spherical space), which results in the universe expanding for a time and then
contracting due to the pull of its gravity in a perpetual cycle of Big Bang followed by Big Crunch Time is thus endless and beginningless, and the beginning-of-time paradox is avoided.

• Steady State Universe - This non-standard cosmology (i.e. opposed to the standard big bang model) has occurred in various versions since the big bang theory was generally
adopted by the scientific community. A popular variant of the steady state universe was proposed in 1948 by the English astronomer Fred Hoyle and the and Austrians Thomas Gold and Hermann
Bondi. It predicted a universe that expanded but did not change its density, with matter being inserted into the universe as it expanded in order to maintain a constant density. Despite its
drawbacks, this was quite a popular idea until the discovery of the cosmic background radiation in 1965 which supported the big bang model

• Inflationary (or Inflating) Universe - In 1980, the American physicist Alan Guth proposed a model of the universe based on the big bang, but incorporating a short,
early period of exponential cosmic inflation in order to solve the horizon and flatness problems of the standard big bang model. Another variation of the inflationary universe is the cyclic model
developed by Paul Steinhardt and Neil Turok in 2002 using state-of-the-art M-theory, superstring theory and brane cosmology, which involves an inflationary universe expanding and contracting in
cycles.

• Multiverse - The Russian-American physicist Andrei Linde developed the inflationary universe idea further in 1983 with his chaotic inflation theory (or internal inflation
which sees our universe as just one of many “bubbles” that grew as part of a multiverse owing to a vacuum that had not decayed to its ground state. The American physicists Hugh Everett III and Bryce
DeWitt had initially developed and popularized their “many worlds” formulation of the multiverse in the 1960s and 1970s. Alternative versions have also been developed where our observable universe is
just one tiny organized part of an infinitely big cosmos which is largely in a state of chaos, or where our organized universe is just one temporary episode in an infinite sequence of largely chaotic
and unorganized arrangements.